Future High Energy Neutrino Telescopes
Astrophysics
2009-10-31 v1
Abstract
This talk summarizes the main physics goals and basic methods of telescopes for high energy neutrinos. It reviews the present status of deep underwater telescopes and sketches the ICECUBE project as an example for a cube kilometer detector. It is suggested to develop techniques for radio and acoustic detection hand in hand with big optical arrays. These large arrays should be complemented by medium-size detectors in the Megaton range.
Cite
@article{arxiv.astro-ph/0012532,
title = {Future High Energy Neutrino Telescopes},
author = {C. Spiering},
journal= {arXiv preprint arXiv:astro-ph/0012532},
year = {2009}
}
Comments
Talk given at the Int.Conf.on Neutrino Physics and Astrophysics, Sudbury 2000, 8 pages, 7 figures